cxprep/chandra.txt: complete registration
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-471L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-471.jpg
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astropix_ids: chandra|471
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credits> NASA/CXC/Wesleyan/R.Kilgard et al.
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---
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@scene
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place_uuid: 8d3ca8d9-de93-4e6d-bead-583c6ec457c4
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-471L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/m82/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-471.jpg
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text> A Chandra image of Messier 82, or M82, shows the result of star formation
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on overdrive. M82 is located about 12 million light years from Earth and is the
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nearest place to us where the conditions are similar to those when the Universe
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was much younger with lots of stars forming.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-472L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-472.jpg
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credits> X-ray (NASA/CXC/Harvard/J.Neilsen et al); Optical (Palomar DSS2)
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---
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@scene
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place_uuid: a4f51693-38ce-43f1-b22d-28a2528c9dea
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-472L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/g1915/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-472.jpg
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text> This optical and infrared image from the Digitized Sky Survey shows the
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crowded field around the binary system GRS 1915+105 (GRS 1915 for short) located
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near the plane of our Galaxy. The top-left inset shows a close-up of the Chandra
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image of GRS 1915 , and the bottom-right inset shows the remarkable "heartbeats"
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seen in the X-ray light from this system. Using Chandra and the Rossi X-ray
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Timing Explorer (RXTE), astronomers have discovered what drives these heartbeats
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and given new insight into the ways that black holes can regulate their intake
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and severely curtail their growth.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-473L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-473.jpg
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astropix_ids: chandra|473
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credits> X-ray (NASA/CXC/Virginia/A.Reines et al); Radio (NRAO/AUI/NSF); Optical
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(NASA/STScI)
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---
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@scene
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place_uuid: 19a5406e-286e-4b0c-825f-55eb4a15ae09
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-473L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/he210/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-473.jpg
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text> The combined observations from multiple telescopes of Henize 2-10, a dwarf
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starburst galaxy located about 30 million light years from Earth, has provided
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astronomers with a detailed new look at how galaxy and black hole formation may
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have occured in the early Universe. This image shows optical data from the
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Hubble Space Telescope in red, green and blue, X-ray data from NASA's Chandra
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X-ray Observatory in purple, and radio data from the National Radio Astronomy
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Observatory's Very Large Array in yellow.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-474L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-474.jpg
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astropix_ids: chandra|474
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credits> X-ray: NASA/CXC/MIT/S.Rappaport et al, Optical: NASA/STScI
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---
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@scene
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place_uuid: d8ef9fdb-f785-41af-bb7b-bfe4cd3639ad
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-474L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/arp147/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-474.jpg
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text> This composite image of Arp 147, a pair of interacting galaxies located
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about 430 million light years from Earth, shows X-rays from the NASA's Chandra
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X-ray Observatory (pink) and optical data from the Hubble Space Telescope (red,
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green, blue) produced by the Space Telescope Science Institute (STScI) in
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Baltimore, MD. Arp 147 contains the remnant of a spiral galaxy that collided
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with an elliptical galaxy.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-476L{1}X{2}Y{3}.png
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copyright: Public domain
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||||
license_id: CC-PDDC
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||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-476.jpg
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astropix_ids: chandra|476
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credits> X-ray: NASA/CXC/UNAM/Ioffe/D.Page,P.Shternin et al; Optical:
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NASA/STScI; Illustration: NASA/CXC/M.Weiss
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---
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@scene
|
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place_uuid: 8a8cc01c-8769-47ca-a7d5-e8a6f85cabc0
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-476L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/casa/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-476.jpg
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text> This composite image shows a beautiful X-ray and optical view of
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Cassiopeia A (Cas A), a supernova remnant located in our Galaxy about 11,000
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light years away. These are the remains of a massive star that exploded about
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330 years ago, as measured in Earth's time frame. X-rays from Chandra are shown
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in red, green and blue along with optical data from Hubble in gold.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-477L{1}X{2}Y{3}.png
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||||
copyright: Public domain
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license_id: CC-PDDC
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||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-477.jpg
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astropix_ids: chandra|477
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credits> X-ray: NASA/CXC/CfA/J.Wang et al.; Optical: Isaac Newton Group of
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Telescopes, La Palma/Jacobus Kapteyn Telescope, Radio: NSF/NRAO/VLA
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|
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---
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@scene
|
||||
place_uuid: 65571ab7-1b26-4ffe-bdbf-f8bfa6693790
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||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-477L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/n4151/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-477.jpg
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text> This composite image shows the central region of the spiral galaxy NGC
|
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4151, dubbed the "Eye of Sauron" by astronomers for its similarity to the eye of
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the malevolent character in "The Lord of the Rings". In the "pupil" of the eye,
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X-rays (blue) from the Chandra X-ray Observatory are combined with optical data
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(yellow) showing positively charged hydrogen ("H II") from observations with the
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1-meter Jacobus Kapteyn Telescope on La Palma.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-478L{1}X{2}Y{3}.png
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||||
copyright: Public domain
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||||
license_id: CC-PDDC
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||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-478.jpg
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astropix_ids: chandra|478
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credits> X-ray: NASA/CXC/Rutgers/K.Eriksen et al.; Optical: DSS
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---
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@scene
|
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place_uuid: 551e84c1-9212-4af0-a725-4b6f10e148a0
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||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-478L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/tycho/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-478.jpg
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text> This image comes from a very deep Chandra observation of the Tycho
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supernova remnant, produced by the explosion of a white dwarf star in our
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Galaxy. Low-energy X-rays (red) in the image show expanding debris from the
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supernova explosion and high energy X-rays (blue) show the blast wave, a shell
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of extremely energetic electrons. These high-energy X-rays show a pattern of
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X-ray "stripes" never previously seen in a supernova remnant.
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---
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@image
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||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-479L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-479.jpg
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astropix_ids: chandra|479
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credits> NASA/CXC/Warwick/A.Levan et al.
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|
||||
---
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@scene
|
||||
place_uuid: 7dbfa8db-78b1-404f-af00-f97496360d75
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-479L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/grb110328/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-479.jpg
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text> The center of this image contains an extraordinary gamma-ray burst (GRB)
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called GRB 110328A, observed with NASA's Chandra X-ray Observatory. This Chandra
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observation confirms the association of GRB 110328A with the core of a distant
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galaxy and shows that it was an exceptionally long lived and luminous event
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compared to other GRBs.
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---
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@image
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||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-480L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-480.jpg
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astropix_ids: chandra|480
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credits> X-ray: NASA/U. of Sydney/G.Anderson et al; IR: NASA/JPL-Caltech
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|
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---
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@scene
|
||||
place_uuid: 5dee1085-aae8-494a-b197-626f4fb90fc4
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||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-480L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/massive/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-480.jpg
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text> Like looking for Easter eggs in a lawn of long grass, the hunt for the
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Milky Way's most massive stars takes persistence and sharp eyes. In their
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stellar search through our Galactic backyard, astronomers have used powerful
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telescopes sensitive to X-ray and infrared radiation to find evidence for a
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substantial population of X-ray emitting massive stars.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-481L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-481.jpg
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astropix_ids: chandra|481
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credits> NASA/CXC/Chinese Academy of Sciences/F. Lu et al.
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---
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@scene
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place_uuid: 78fedc1b-453d-4e33-baeb-f0b307f0631b
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||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-481L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/tycho2/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-481.jpg
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text> This new image of Tycho's supernova remnant, dubbed Tycho for short,
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contains striking new evidence for what triggered the original supernova
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explosion, as seen from Earth in 1572. Tycho was formed by a Type Ia supernova,
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a category of stellar explosion used in measuring astronomical distances because
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of their reliable brightness.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-483L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-483.jpg
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astropix_ids: chandra|483
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credits> NASA/CXC/PSU/L.Townsley et al.
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---
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@scene
|
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place_uuid: cce0525c-4d04-4c45-bd77-b0252f9088c8
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image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-483L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/carina/more.html#img1c
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-483.jpg
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text> This Chandra image is 22 separate pointings of the telescope that have
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been stitched together to look at the famous Carina Nebula like never before. In
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this image, low, medium, and high-energy X-rays are colored red, green, and blue
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respectively. Chandra detected over 14,000 stars in this region, revealed a
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diffuse X-ray glow, and provided strong evidence that massive stars have already
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self-destructed in this nearby supernova factory. The Carina Nebula is one of
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the best places in the Milky Way to study how young and massive stars live and
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die.
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---
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@image
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url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-484L{1}X{2}Y{3}.png
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copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-484.jpg
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astropix_ids: chandra|484
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credits> X-ray: NASA/CXC/U.Hawaii/E.Treister et al; Infrared: NASA/STScI/UC
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Santa Cruz/G.Illingworth et al; Optical: NASA/STScI/S.Beckwith et al
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---
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@scene
|
||||
place_uuid: 8461475c-4078-4e8b-865a-9c9ec39fd13c
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-484L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/cdfs/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-484.jpg
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text> This composite image from NASA's Chandra X-ray Observatory and Hubble
|
||||
Space Telescope (HST) combines the deepest X-ray, optical and infrared views of
|
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the sky. Astronomers obtained what is known as the Chandra Deep Field South
|
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(CDFS) by pointing the telescope at the same patch of sky for over six weeks of
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time. The composite image shows a small section of the CDFS, where the Chandra
|
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sources are blue, the optical HST data are shown in green and blue, and the
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infrared data from Hubble are in red and green.
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---
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@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-485L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-485.jpg
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astropix_ids: chandra|485
|
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|
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credits> X-ray: NASA/CXC/ITA/INAF/J.Merten et al, Lensing: NASA/STScI;
|
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NAOJ/Subaru; ESO/VLT, Optical: NASA/STScI/R.Dupke
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|
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---
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@scene
|
||||
place_uuid: 601ecafb-1632-4f18-8c56-73b5e3709192
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-485L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/a2744/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-485.jpg
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text> One of the most complicated and dramatic collisions between galaxy
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clusters ever seen is captured in this new composite image. This collision site,
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known officially as Abell 2744, has been dubbed "Pandora's Cluster" because of
|
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the wide variety of different structures seen. Data from NASA's Chandra X-ray
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Observatory are colored red, showing gas with temperatures of millions of
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degrees.
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---
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@image
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||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-486L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-486.jpg
|
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astropix_ids: chandra|486
|
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|
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credits> X-ray: NASA/CXC/IUSS/A.De Luca et al; Optical: DSS
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---
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||||
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@scene
|
||||
place_uuid: 6f84278a-8539-42a1-92e6-55ec76258068
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-486L{1}X{2}Y{3}.png
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outgoing_url: https://chandra.harvard.edu/photo/2011/psrj0357/
|
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-486.jpg
|
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|
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text> A spinning neutron star is tied to a mysterious tail - or so it seems.
|
||||
Astronomers using NASA's Chandra X-ray Observatory have found that this pulsar,
|
||||
known as PSR J0357+3205 (or PSR J0357 for short), apparently has a long, X-ray
|
||||
bright tail streaming away from it.
|
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|
||||
---
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|
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@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-487L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-487.jpg
|
||||
astropix_ids: chandra|487
|
||||
|
||||
credits> X-ray: NASA/CXC/Univ. of Alabama/K.Wong et al, Optical: ESO/VLT
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 82a27eb0-9692-48ea-a5b2-0f40b32fe264
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-487L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2011/n3115/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-487.jpg
|
||||
|
||||
text> The galaxy NGC 3115 is shown here in a composite image of data from NASA's
|
||||
Chandra X-ray Observatory and the European Southern Observatory's Very Large
|
||||
Telescope (VLT). Using the Chandra image, the flow of hot gas toward the
|
||||
supermassive black hole in the center of this galaxy has been imaged. This is
|
||||
the first time that clear evidence for such a flow has been observed in any
|
||||
black hole.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-488L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-488.jpg
|
||||
astropix_ids: chandra|488
|
||||
|
||||
credits> X-ray NASA/CXC/IfA/D.Sanders et al; Optical NASA/STScI/NRAO/A.Evans et
|
||||
al
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: b6bdc127-362a-497d-9ef6-32a6191b1018
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-488L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2011/vv340/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-488.jpg
|
||||
|
||||
text> VV 340, also known as Arp 302, provides a textbook example of colliding
|
||||
galaxies seen in the early stages of their interaction. The edge-on galaxy near
|
||||
the top of the image is VV 340 North and the face-on galaxy at the bottom of the
|
||||
image is VV 340 South. Millions of years later these two spirals will merge —
|
||||
much like the Milky Way and Andromeda will likely do billions of years from now.
|
||||
Data from NASA's Chandra X-ray Observatory (purple) are shown here along with
|
||||
optical data from the Hubble Space Telescope (red, green, blue). VV 340 is
|
||||
located about 450 million light years from Earth.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-489L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-489.jpg
|
||||
astropix_ids: chandra|489
|
||||
|
||||
credits> X-ray: NASA/CXC/SAO/G.Fabbiano et al; Optical: NASA/STScI
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: ec2b9585-5971-4906-9d62-0f18e1b3893f
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-489L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2011/n3393/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-489.jpg
|
||||
|
||||
text> Evidence for a pair of supermassive black holes in a spiral galaxy has
|
||||
been found in data from NASA's Chandra X-ray Observatory. This main image is a
|
||||
composite of X-rays from Chandra (blue) and optical data from the Hubble Space
|
||||
Telescope (gold) of the spiral galaxy NGC 3393. Meanwhile, the inset box shows
|
||||
the central region of NGC 3993 as observed just by Chandra.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-491L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-491.jpg
|
||||
astropix_ids: chandra|491
|
||||
|
||||
credits> X-ray: NASA/CXC/CfA/S.Wolk; IR: NASA/JPL/CfA/S.Wolk
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 392352c2-fa94-4dbe-9d4d-2724fdf74de3
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-491L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2011/ngc281/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-491.jpg
|
||||
|
||||
text> High-mass stars are important because they are responsible for much of the
|
||||
energy pumped into our galaxy over its lifetime. Unfortunately, these stars are
|
||||
poorly understood because they are often found relatively far away and can be
|
||||
obscured by gas and dust. The star cluster NGC 281 is an exception to this rule.
|
||||
It is located about 9,200 light years from Earth and, remarkably, almost 1,000
|
||||
light years above the plane of the Galaxy, giving astronomers a nearly
|
||||
unfettered view of the star formation within it.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-492L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-492.jpg
|
||||
astropix_ids: chandra|492
|
||||
|
||||
credits> X-ray: NASA/CXC/U. Texas at Arlington/S.Park et al, ROSAT; Infrared:
|
||||
2MASS/UMass/IPAC-Caltech/NASA/NSF
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 82c1feb7-d388-45a8-9840-1976d7ffcb42
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-492L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2011/g299/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-492.jpg
|
||||
|
||||
text> G299.2-2.9 is an intriguing supernova remnant found about 16,000 light
|
||||
years away in the Milky Way galaxy. Evidence points to G299.2-2.9 being the
|
||||
remains of a Type Ia supernova, where a white dwarf has grown sufficiently
|
||||
massive to cause a thermonuclear explosion. Because it is older than most
|
||||
supernova remnants caused by these explosions, at an age of about 4500 years,
|
||||
G299.2-2.9 provides astronomers with an excellent opportunity to study how these
|
||||
objects evolve over time. It also provides a probe of the Type Ia supernova
|
||||
explosion that produced this structure.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-494L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-494.jpg
|
||||
astropix_ids: chandra|494
|
||||
|
||||
credits> X-ray: NASA/CXC/SAO & ESA; Infared: NASA/JPL-Caltech/B. Williams (NCSU)
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 5fc6778d-612b-4077-96ae-c303df6fdd68
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-494L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2011/rcw86/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-494.jpg
|
||||
|
||||
text> This image combines data from four different space telescopes to create a
|
||||
multi-wavelength view of all that remains of the oldest documented example of a
|
||||
supernova, called RCW 86. The Chinese witnessed the event in 185 A.D.,
|
||||
documenting a mysterious "guest star" that remained in the sky for eight months.
|
||||
X-ray images from NASA's Chandra X-ray Observatory and the European Space
|
||||
Agency's XMM-Newton Observatory are combined to form the blue and green colors
|
||||
in the image. The X-rays show the interstellar gas that has been heated to
|
||||
millions of degrees by the passage of the shock wave from the supernova.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-495L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-495.jpg
|
||||
astropix_ids: chandra|495
|
||||
|
||||
credits> X-ray: NASA/CXC/PSU/L.Townsley et al.; Infrared: NASA/JPL/PSU/L.Townsley et al.
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 19d149aa-0183-4d66-8ca1-8b0419050fe5
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-495L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2011/30dor/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-495.jpg
|
||||
|
||||
text> The star-forming region, 30 Doradus, is one of the largest located close
|
||||
to the Milky Way and is found in the neighboring galaxy Large Magellanic Cloud.
|
||||
About 2,400 massive stars in the center of 30 Doradus, also known as the
|
||||
Tarantula Nebula, are producing intense radiation and powerful winds as they
|
||||
blow off material.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-497L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-497.jpg
|
||||
astropix_ids: chandra|497
|
||||
|
||||
credits> X-ray: NASA/CXC/BU/E.Blanton; Optical: ESO/VLT
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 6fdede50-fa87-4191-8bcc-533713fa7206
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-497L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2011/a2052/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-497.jpg
|
||||
|
||||
text> Like wine in a glass, vast clouds of hot gas are sloshing back and forth
|
||||
in Abell 2052, a galaxy cluster located about 480 million light years from
|
||||
Earth. X-ray data (blue) from NASA's Chandra X-ray Observatory shows the hot gas
|
||||
in this dynamic system, and optical data (gold) from the Very Large Telescope
|
||||
shows the galaxies. The hot, X-ray bright gas has an average temperature of
|
||||
about 30 million degrees.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-498L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-498.jpg
|
||||
astropix_ids: chandra|498
|
||||
|
||||
credits> X-ray: NASA/CXC/Univ.Potsdam/L.Oskinova et al & ESA/XMM-Newton; Optical: AURA/NOAO/CTIO/Univ.Potsdam/L.Oskinova et al
|
||||
|
||||
---
|
||||
|
||||
@scene
|
||||
place_uuid: 64314825-092c-4925-a492-233d5f65f533
|
||||
image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-498L{1}X{2}Y{3}.png
|
||||
outgoing_url: https://chandra.harvard.edu/photo/2011/sxp1062/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-498.jpg
|
||||
|
||||
text> Data from NASA's Chandra X-ray Observatory and ESA's XMM-Newton have been
|
||||
combined to discover a young pulsar in the remains of a supernova located in the
|
||||
Small Magellanic Cloud, or SMC. This would be the first definite time a pulsar,
|
||||
a spinning, ultra-dense star, has been found in a supernova remnant in the SMC,
|
||||
a small satellite galaxy to the Milky Way. The pulsar, known as SXP 1062, is the
|
||||
bright white source located on the right-hand side of the image in the middle of
|
||||
the diffuse blue emission inside a red shell.
|
||||
|
||||
---
|
||||
|
||||
@image
|
||||
url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-499L{1}X{2}Y{3}.png
|
||||
copyright: Public domain
|
||||
|
|
|
|||
|
|
@ -50612,7 +50612,7 @@ powers the dramatic activity seen by...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-471L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|471"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0db01d08292018533b5"
|
||||
>
|
||||
<Credits>NASA/CXC/Wesleyan/R.Kilgard et a; M82 is a galaxy where stars are forming at rates that are tens or even hundreds of times higher than in a normal galaxy. In this...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/m82/</CreditsUrl>
|
||||
|
|
@ -50638,7 +50638,7 @@ powers the dramatic activity seen by...</Credits>
|
|||
TileLevels="4"
|
||||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-472L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0dc01d08292018533b7"
|
||||
>
|
||||
<Credits>X-ray (NASA/CXC/Harvard/J.Neilsen et al); Optical (Palomar DSS2)</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/g1915/</CreditsUrl>
|
||||
|
|
@ -50665,7 +50665,7 @@ powers the dramatic activity seen by...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-473L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|473"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0dd01d08292018533b9"
|
||||
>
|
||||
<Credits>X-ray (NASA/CXC/Virginia/A.Reine; Combined observations from Chandra (purple), the Very Large Array (yellow) along with Hubble (red, green, and blue) have provide...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/he210/</CreditsUrl>
|
||||
|
|
@ -50692,7 +50692,7 @@ powers the dramatic activity seen by...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-474L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|474"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0de01d08292018533bb"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/MIT/S.Rappaport et al, Optical: NASA/STScI</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/arp147/</CreditsUrl>
|
||||
|
|
@ -50719,7 +50719,7 @@ powers the dramatic activity seen by...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-476L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|476"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0df01d08292018533bd"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/UNAM/Ioffe/D.Page,P.Shternin et al; Optical: NASA/STScI; Illustration: NASA/CXC/M.Weiss</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/casa/</CreditsUrl>
|
||||
|
|
@ -50746,7 +50746,7 @@ powers the dramatic activity seen by...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-477L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|477"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0e001d08292018533bf"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/CfA/J.Wang et al.; Optical: Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope, Radio: NSF/NRAO/VLA</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/n4151/</CreditsUrl>
|
||||
|
|
@ -50773,7 +50773,7 @@ powers the dramatic activity seen by...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-478L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|478"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0e101d08292018533c1"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Rutgers/K.Erikse; A long Chandra observation of Tycho has revealed a pattern
|
||||
of X-ray stripes never seen before in a supernova remnant. The
|
||||
|
|
@ -50802,7 +50802,7 @@ s...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-479L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|479"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0e201d08292018533c3"
|
||||
>
|
||||
<Credits>NASA/CXC/Warwick/A.Levan et al.; The center of this image contains an extraordinary gamma-ray burst (GRB 110328A) observed with Chandra. The burst was first seen...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/grb110328/</CreditsUrl>
|
||||
|
|
@ -50829,7 +50829,7 @@ s...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-480L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|480"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0e301d08292018533c5"
|
||||
>
|
||||
<Credits>X-ray: NASA/U. of Sydney/G.Ander; Data from Chandra and Spitzer of a region near the Galactic
|
||||
plane have been combined to track down some of the Milky Way's
|
||||
|
|
@ -50858,7 +50858,7 @@ h...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-481L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|481"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0e401d08292018533c7"
|
||||
>
|
||||
<Credits>NASA/CXC/Chinese Academy of Scie; This Chandra image of the Tycho supernova remnant contains new evidence for what triggered the original supernova explosion. Ty...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/tycho2/</CreditsUrl>
|
||||
|
|
@ -50912,7 +50912,7 @@ h...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-483L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|483"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0e501d08292018533c9"
|
||||
>
|
||||
<Credits>NASA/CXC/PSU/L.Townsley et al.</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/carina/more.html#img1c</CreditsUrl>
|
||||
|
|
@ -50939,7 +50939,7 @@ h...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-484L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|484"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0e601d08292018533cb"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/U.Hawaii/E.Treis; This composite image combines the deepest X-ray image ever taken with optical and infrared data from Hubble. Astronomers obtain...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/cdfs/</CreditsUrl>
|
||||
|
|
@ -50966,7 +50966,7 @@ h...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-485L{1}X{2}Y{3}.png"
|
||||
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|
||||
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|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0e701d08292018533cd"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/ITA/INAF/J.Merte; This composite image features one of the most complicated and dramatic collisions between galaxy clusters ever seen. Known off...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/a2744/</CreditsUrl>
|
||||
|
|
@ -50993,7 +50993,7 @@ h...</Credits>
|
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Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-486L{1}X{2}Y{3}.png"
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|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0e801d08292018533cf"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/IUSS/A.De Luca e; Astronomers using Chandra have found evidence for a possible long, X- ray bright tail extending from the pulsar called PSR J0357...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/psrj0357/</CreditsUrl>
|
||||
|
|
@ -51020,7 +51020,7 @@ h...</Credits>
|
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Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-487L{1}X{2}Y{3}.png"
|
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|
||||
Xcxstatus="queue:chandra"
|
||||
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|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/Univ. of Alabama; This composite image contains X-rays from Chandra (blue) and optical data from the VLT (gold) of the galaxy NGC 3115. Using the...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/n3115/</CreditsUrl>
|
||||
|
|
@ -51047,7 +51047,7 @@ h...</Credits>
|
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Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-488L{1}X{2}Y{3}.png"
|
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|
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|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0ea01d08292018533d3"
|
||||
>
|
||||
<Credits>X-ray NASA/CXC/IfA/D.Sanders et ; This composite image of VV 340 contains X-ray data from Chandra (purple)
|
||||
and optical data from Hubble (red, green, blue). The tw...</Credits>
|
||||
|
|
@ -51075,7 +51075,7 @@ and optical data from Hubble (red, green, blue). The tw...</Credits>
|
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Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-489L{1}X{2}Y{3}.png"
|
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|
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|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0eb01d08292018533d5"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/SAO/G.Fabbiano e; Evidence for a pair of supermassive black holes in a spiral
|
||||
galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
||||
|
|
@ -51103,7 +51103,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-491L{1}X{2}Y{3}.png"
|
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|
||||
Xastropix_ids="chandra|491"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0ec01d08292018533d7"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/CfA/S.Wolk; IR: ; This composite image of NGC 281 contains X-ray data from Chandra (purple) with infrared observations from Spitzer (red, green, b...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/ngc281/</CreditsUrl>
|
||||
|
|
@ -51130,7 +51130,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-492L{1}X{2}Y{3}.png"
|
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|
||||
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|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0ed01d08292018533d9"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/U. Texas at Arlington/S.Park et al, ROSAT; Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSF</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/g299/</CreditsUrl>
|
||||
|
|
@ -51157,7 +51157,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-494L{1}X{2}Y{3}.png"
|
||||
WidthFactor="1"
|
||||
Xastropix_ids="chandra|494"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0ed01d08292018533db"
|
||||
>
|
||||
<Credits>NASA/JPL-Caltech/B. Williams (NC; This image combines data from four different space telescopes to create a multi-wavelength view of all that remains of the oldes...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/rcw86/</CreditsUrl>
|
||||
|
|
@ -51184,7 +51184,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
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Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-495L{1}X{2}Y{3}.png"
|
||||
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|
||||
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|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0ee01d08292018533dd"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/PSU/L.Townsley e; About 2,400 massive stars in the center of 30 Doradus are producing intense radiation and powerful winds as they blow off materi...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/30dor/</CreditsUrl>
|
||||
|
|
@ -51211,7 +51211,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-497L{1}X{2}Y{3}.png"
|
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WidthFactor="1"
|
||||
Xastropix_ids="chandra|497"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0ef01d08292018533df"
|
||||
>
|
||||
<Credits>X-ray: NASA/CXC/BU/E.Blanton; Optical: ESO/VLT</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/a2052/</CreditsUrl>
|
||||
|
|
@ -51238,7 +51238,7 @@ galaxy has been found in data from NASA's Chandra X-ray Observator...</Credits>
|
|||
Url="http://wwtfiles.blob.core.windows.net/vamp/Chandra-498L{1}X{2}Y{3}.png"
|
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WidthFactor="1"
|
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Xastropix_ids="chandra|498"
|
||||
Xcxstatus="queue:chandra"
|
||||
Xcxstatus="in:66c4a0f001d08292018533e1"
|
||||
>
|
||||
<Credits>X-ray & Optical: NASA/CXC/Univ.P; In this composite image, X-rays from Chandra and XMM-Newton (blue) have been combined with optical data from the Cerro Tololo In...</Credits>
|
||||
<CreditsUrl>https://chandra.harvard.edu/photo/2011/sxp1062/</CreditsUrl>
|
||||
|
|
|
|||
|
|
@ -1679,8 +1679,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-454.jpg
|
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zoom_level: 3.49970317312
|
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---
|
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|
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astropix_id: chandra|478
|
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classification: ''
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constellation: CAS
|
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cxstatus: in:66c4a0e101d08292018533c2
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dec_deg: 64.1385494
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|
||||
|
|
@ -1690,8 +1692,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-478.jpg
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zoom_level: 1.444427087872
|
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---
|
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|
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astropix_id: chandra|481
|
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classification: ''
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constellation: CAS
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cxstatus: in:66c4a0e501d08292018533c8
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data_set_type: Sky
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dec_deg: 64.1385494
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-481L{1}X{2}Y{3}.png
|
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|
|
@ -1701,8 +1705,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-481.jpg
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zoom_level: 1.14109739941888
|
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---
|
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astropix_id: chandra|485
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constellation: SCL
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cxstatus: in:66c4a0e701d08292018533ce
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-485L{1}X{2}Y{3}.png
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|
|
@ -1712,8 +1718,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-485.jpg
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zoom_level: 0.509527588864
|
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---
|
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astropix_id: chandra|491
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constellation: CAS
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cxstatus: in:66c4a0ec01d08292018533d8
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dec_deg: 56.594963
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-491L{1}X{2}Y{3}.png
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|
|
|
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|
|
@ -1222,8 +1222,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-431.jpg
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zoom_level: 0.216174788608
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---
|
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astropix_id: chandra|498
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constellation: HYI
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cxstatus: in:66c4a0f101d08292018533e2
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-498L{1}X{2}Y{3}.png
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|
|
|
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|
|
@ -1883,8 +1883,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-443.jpg
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zoom_level: 0.2320171008
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---
|
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astropix_id: chandra|474
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constellation: CET
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cxstatus: in:66c4a0de01d08292018533bc
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data_set_type: Sky
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dec_deg: 1.3143841
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-474L{1}X{2}Y{3}.png
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|
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@ -1894,8 +1896,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-474.jpg
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zoom_level: 0.0680777465856
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---
|
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astropix_id: chandra|484
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constellation: FOR
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cxstatus: in:66c4a0e601d08292018533cc
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-484L{1}X{2}Y{3}.png
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|
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@ -1905,8 +1909,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-484.jpg
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zoom_level: 0.166325247363728
|
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---
|
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astropix_id: chandra|486
|
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cxstatus: in:66c4a0e801d08292018533d0
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-486L{1}X{2}Y{3}.png
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|
|
|
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|
|
@ -4686,8 +4686,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-482.jpg
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zoom_level: 0.234100297728
|
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---
|
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astropix_id: chandra|495
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constellation: DOR
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-495L{1}X{2}Y{3}.png
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|
|
|
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|
|
@ -538,8 +538,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-470.jpg
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zoom_level: 1.40640760004877
|
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---
|
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astropix_id: chandra|473
|
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classification: ''
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constellation: PYX
|
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cxstatus: in:66c4a0dd01d08292018533ba
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-473L{1}X{2}Y{3}.png
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|
|
|
|||
|
|
@ -715,8 +715,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-434.jpg
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zoom_level: 0.748183552
|
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---
|
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|
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constellation: UMA
|
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cxstatus: in:66c4a0db01d08292018533b6
|
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-471L{1}X{2}Y{3}.png
|
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|
|
|
|||
|
|
@ -1561,8 +1561,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-456.jpg
|
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zoom_level: 0.0569144344576
|
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---
|
||||
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|
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|
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|
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|
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-483L{1}X{2}Y{3}.png
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|
|
@ -1572,8 +1574,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-483.jpg
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zoom_level: 7.7107265536
|
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---
|
||||
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|
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|
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|
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-487L{1}X{2}Y{3}.png
|
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|
|
@ -1583,8 +1587,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-487.jpg
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zoom_level: 0.567366664192
|
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---
|
||||
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|
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|
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|
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foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-489L{1}X{2}Y{3}.png
|
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|
|
|
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|
|
@ -2815,8 +2815,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-467.jpg
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zoom_level: 0.390792511488
|
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---
|
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|
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|
|
@ -2826,8 +2828,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-477.jpg
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|
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---
|
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|
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|
|
|
|||
|
|
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|
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---
|
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|
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|
|
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---
|
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|
||||
astropix_id: chandra|488
|
||||
classification: ''
|
||||
constellation: BOO
|
||||
cxstatus: in:66c4a0ea01d08292018533d4
|
||||
data_set_type: Sky
|
||||
dec_deg: 24.6131728
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-488L{1}X{2}Y{3}.png
|
||||
|
|
@ -897,8 +901,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-488.jpg
|
|||
zoom_level: 0.167625392128
|
||||
---
|
||||
_uuid: 5fc6778d-612b-4077-96ae-c303df6fdd68
|
||||
astropix_id: chandra|494
|
||||
classification: ''
|
||||
constellation: CIR
|
||||
cxstatus: in:66c4a0ee01d08292018533dc
|
||||
data_set_type: Sky
|
||||
dec_deg: -62.4631333802834
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-494L{1}X{2}Y{3}.png
|
||||
|
|
|
|||
|
|
@ -472,8 +472,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-468.jpg
|
|||
zoom_level: 0.894903451648
|
||||
---
|
||||
_uuid: 6fdede50-fa87-4191-8bcc-533713fa7206
|
||||
astropix_id: chandra|497
|
||||
classification: ''
|
||||
constellation: SER1
|
||||
cxstatus: in:66c4a0f001d08292018533e0
|
||||
data_set_type: Sky
|
||||
dec_deg: 7.0215835
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-497L{1}X{2}Y{3}.png
|
||||
|
|
|
|||
|
|
@ -1340,8 +1340,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-458.jpg
|
|||
zoom_level: 1.19196168415418
|
||||
---
|
||||
_uuid: 7dbfa8db-78b1-404f-af00-f97496360d75
|
||||
astropix_id: chandra|479
|
||||
classification: ''
|
||||
constellation: DRA
|
||||
cxstatus: in:66c4a0e201d08292018533c4
|
||||
data_set_type: Sky
|
||||
dec_deg: 57.583278
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-479L{1}X{2}Y{3}.png
|
||||
|
|
|
|||
|
|
@ -1409,8 +1409,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-455.jpg
|
|||
zoom_level: 0.9076298612736
|
||||
---
|
||||
_uuid: a4f51693-38ce-43f1-b22d-28a2528c9dea
|
||||
astropix_id: null
|
||||
classification: ''
|
||||
constellation: AQL
|
||||
cxstatus: in:66c4a0dc01d08292018533b8
|
||||
data_set_type: Sky
|
||||
dec_deg: 11.300081423
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-472L{1}X{2}Y{3}.png
|
||||
|
|
|
|||
|
|
@ -1074,8 +1074,10 @@ thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-463.jpg
|
|||
zoom_level: 1.03486538621673
|
||||
---
|
||||
_uuid: 8a8cc01c-8769-47ca-a7d5-e8a6f85cabc0
|
||||
astropix_id: chandra|476
|
||||
classification: ''
|
||||
constellation: CAS
|
||||
cxstatus: in:66c4a0df01d08292018533be
|
||||
data_set_type: Sky
|
||||
dec_deg: 58.814723
|
||||
foreground_image_set_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-476L{1}X{2}Y{3}.png
|
||||
|
|
|
|||
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